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dc.contributor.authorCMS Collaboration
dc.date.accessioned2023-08-16T18:08:36Z
dc.date.available2023-08-16T18:08:36Z
dc.date.issued2023-07-03
dc.identifier.citationTumasyan, A., Adam, W., Andrejkovic, J.W. et al. Measurement of the differential tt⎯⎯ production cross section as a function of the jet mass and extraction of the top quark mass in hadronic decays of boosted top quarks. Eur. Phys. J. C 83, 560 (2023). https://doi.org/10.1140/epjc/s10052-023-11587-8en_US
dc.identifier.urihttps://hdl.handle.net/1808/34744
dc.description.abstractA measurement of the jet mass distribution in hadronic decays of Lorentz-boosted top quarks is presented. The measurement is performed in the lepton + jets channel of top quark pair production (tt⎯⎯) events, where the lepton is an electron or muon. The products of the hadronic top quark decay are reconstructed using a single large-radius jet with transverse momentum greater than 400GeV. The data were collected with the CMS detector at the LHC in proton-proton collisions and correspond to an integrated luminosity of 138fb−1. The differential tt⎯⎯ production cross section as a function of the jet mass is unfolded to the particle level and is used to extract the top quark mass. The jet mass scale is calibrated using the hadronic W boson decay within the large-radius jet. The uncertainties in the modeling of the final state radiation are reduced by studying angular correlations in the jet substructure. These developments lead to a significant increase in precision, and a top quark mass of 173.06±0.84GeV.en_US
dc.publisherElsevieren_US
dc.rights© CERN for the benefit of the CMS collaboration 2023. This article is licensed under a Creative Commons Attribution 4.0 International License.en_US
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/en_US
dc.titleMeasurement of the differential tt⎯⎯ production cross section as a function of the jet mass and extraction of the top quark mass in hadronic decays of boosted top quarksen_US
dc.typeArticleen_US
kusw.kuauthorAbreu, A.
kusw.kuauthorAlcerro Alcerro, L. F.
kusw.kuauthorAnguiano, J.
kusw.kuauthorBaringer, P.
kusw.kuauthorBean, A.
kusw.kuauthorFlowers, Z.
kusw.kuauthorIsidori, T.
kusw.kuauthorKing, J.
kusw.kuauthorKrintiras, G.
kusw.kuauthorLazarovits, M.
kusw.kuauthorLe Mahieu, C.
kusw.kuauthorLindsey, C.
kusw.kuauthorMarquez, J.
kusw.kuauthorMinafra, N.
kusw.kuauthorMurray, M.
kusw.kuauthorNickel, M.
kusw.kuauthorRogan, C.
kusw.kuauthorRoyon, C.
kusw.kuauthorSalvatico, R.
kusw.kuauthorSanders, S.
kusw.kuauthorSmith, C.
kusw.kuauthorWang, Q.
kusw.kuauthorWilliams, J.
kusw.kuauthorWilson, G.
kusw.kudepartmentPhysics & Astronomyen_US
dc.identifier.doi10.1140/epjc/s10052-023-11587-8en_US
kusw.oaversionScholarly/refereed, publisher versionen_US
kusw.oapolicyThis item meets KU Open Access policy criteria.en_US
dc.identifier.pmidPMC10317917en_US
dc.rights.accessrightsopenAccessen_US


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© CERN for the benefit of the CMS collaboration 2023. This article is licensed under a Creative Commons Attribution 4.0 International License.
Except where otherwise noted, this item's license is described as: © CERN for the benefit of the CMS collaboration 2023. This article is licensed under a Creative Commons Attribution 4.0 International License.